Hubble Law and Brane Matter after Ekpyrosis
arXiv:hep-th/0106282 · doi:10.1016/S0550-3213(01)00412-6
Abstract
We study brane matter in the ekpyrotic scenario and observe that in order to obtain standard gravity on the visible brane, the tension of the visible brane should be positive. If the sizes of both the fifth dimension and the Calabi-Yau threefold are fixed, the Israel junction conditions do not allow time-dependent brane matter. Relaxing this constraint, it is possible to obtain approximately standard cosmology on the visible brane, with small corrections due to possible time-dependence of the Calabi-Yau threefold.
17 pages, LaTex2e. v2: References added, discussion clarified. v3: Summary of tension debate revised, wordings clarified
References in corpus (1)
Cited by in corpus (13)
- On the Generation of a Scale-Invariant Spectrum of Adiabatic Fluctuations in Cosmological Models with a Contracting Phase
- A Critical Review of Classical Bouncing Cosmologies
- On the Construction of Nonsingular Pre-Big-Bang and Ekpyrotic Cosmologies and the Resulting Density Perturbations
- Adiabatic perturbations in pre big bang models: matching conditions and scale invariance
- Cosmological structure problem of the ekpyrotic scenario
- Comment on "Density perturbations in the ekpyrotic scenario"
- Perturbations in a Bouncing Brane Model
- On ekpyrotic brane collisions
- Five Dimensional Cosmology in Horava-Witten M-Theory
- From Big Crunch to Big Bang: A Quantum String Cosmology Perspective
- Gravitational Forces in the Randall-Sundrum Model with a Scalar Stabilizing Field
- Time-dependent toroidal compactification proposals and the Bianchi type II model: classical and quantum solutions
- Gravitational Forces in the Brane World